Professor Rob Fender: Publications

An artist's impression of a relativistic jet propagating away from a black hole at close to the speed of light. Such jets are formed by the inner regions of the accretion flow: matter flowing inwards towards the black hole, via processes which are not yet fully understood. The accretion flow emits primarily in X-rays, the relativistic jet in the radio band: by combing observations in each band we can try and understand how such jets form and how much energy they carry away from the black hole.

The infrared counterpart of the Z source GX5-1

(2000)

Authors:

Peter G Jonker, Rob P Fender, Nigel C Hambly, Michiel van der Klis

Orbital dynamics of Cygnus X-3

(2000)

Authors:

MM Hanson, MD Still, RP Fender

Resolving the radio nebula around beta Lyrae

(2000)

Authors:

G Umana, PFL Maxted, C Trigilio, RP Fender, F Leone, SK Yerli

Excess sub-millimetre emission from GRS 1915+105

(2000)

Authors:

RN Ogley, SJ Bell Burnell, RP Fender, GG Pooley, EB Waltman

Identification of a Likely Radio Counterpart to the Rapid Burster

The Astrophysical Journal American Astronomical Society 532:2 (2000) 1181-1191

Authors:

Christopher B Moore, Robert E Rutledge, Derek W Fox, Robert A Guerriero, Walter HG Lewin, Robert Fender, Jan van Paradijs

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